English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

The extensivity for the thermodynamics of general $D$-dimensional rotatingblack holes with or without a cosmological constant can be proved analytically,provided the effective number of microscopic degrees of freedom and thechemical potential are given respectively as $N=L^{D-2}/G, \mu= GTI_D/L^{D-2}$,where $G$ is the variable Newton constant, $I_D$ is the Euclidean action and$L$ is a constant length scale. In the cases without a cosmological constant,i.e. the Myers-Perry black holes, the physical mass and the intensive variablescan be expressed as explicit macro state functions in the extensive variablesin a simple and compact form, which allows for an analytical calculation forthe heat capacity. The results indicate that the Myers-Perry black holes withzero, one and $k$ equal rotation parameters are all thermodynamically unstable.

Thermodynamics for higher dimensional rotating black holes with variable Newton constant